Results from the Super Cryogenic Dark Matter Search Experiment at Soudan
We report the result of a blinded search for weakly interacting massive particles (WIMPs) using the majority of the SuperCDMS Soudan data set. With an exposure of 1690 kg d, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results)...
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| Veröffentlicht in: | Physical review letters 2018-02, Vol.120 (6), p.061802-061802, Article 061802 |
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| creator | Agnese, R Aramaki, T Arnquist, I J Baker, W Balakishiyeva, D Banik, S Barker, D Basu Thakur, R Bauer, D A Binder, T Bowles, M A Brink, P L Bunker, R Cabrera, B Caldwell, D O Calkins, R Cartaro, C Cerdeño, D G Chang, Y Chen, Y Cooley, J Cornell, B Cushman, P Daal, M Di Stefano, P C F Doughty, T Fascione, E Figueroa-Feliciano, E Fritts, M Gerbier, G Germond, R Ghaith, M Godfrey, G L Golwala, S R Hall, J Harris, H R Hong, Z Hoppe, E W Hsu, L Huber, M E Iyer, V Jardin, D Jastram, A Jena, C Kelsey, M H Kennedy, A Kubik, A Kurinsky, N A Loer, B Lopez Asamar, E Lukens, P MacDonell, D Mahapatra, R Mandic, V Mast, N Miller, E H Mirabolfathi, N Mohanty, B Morales Mendoza, J D Nelson, J Orrell, J L Oser, S M Page, K Page, W A Partridge, R Penalver Martinez, M Pepin, M Phipps, A Poudel, S Pyle, M Qiu, H Rau, W Redl, P Reisetter, A Reynolds, T Roberts, A Robinson, A E Rogers, H E Saab, T Sadoulet, B Sander, J Schneck, K Schnee, R W Scorza, S Senapati, K Serfass, B Speller, D Stein, M Street, J Tanaka, H A Toback, D Underwood, R Villano, A N von Krosigk, B Welliver, B Wilson, J S Wilson, M J Wright, D H Yellin, S Yen, J J |
| description | We report the result of a blinded search for weakly interacting massive particles (WIMPs) using the majority of the SuperCDMS Soudan data set. With an exposure of 1690 kg d, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP-nucleon cross section of 1.4×10^{-44} (1.0×10^{-44}) cm^{2} at 46 GeV/c^{2}. These results set the strongest limits for WIMP-germanium-nucleus interactions for masses >12 GeV/c^{2}. |
| doi_str_mv | 10.1103/PhysRevLett.120.061802 |
| format | Article |
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With an exposure of 1690 kg d, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP-nucleon cross section of 1.4×10^{-44} (1.0×10^{-44}) cm^{2} at 46 GeV/c^{2}. 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P</creatorcontrib><creatorcontrib>Reisetter, A</creatorcontrib><creatorcontrib>Reynolds, T</creatorcontrib><creatorcontrib>Roberts, A</creatorcontrib><creatorcontrib>Robinson, A E</creatorcontrib><creatorcontrib>Rogers, H E</creatorcontrib><creatorcontrib>Saab, T</creatorcontrib><creatorcontrib>Sadoulet, B</creatorcontrib><creatorcontrib>Sander, J</creatorcontrib><creatorcontrib>Schneck, K</creatorcontrib><creatorcontrib>Schnee, R W</creatorcontrib><creatorcontrib>Scorza, S</creatorcontrib><creatorcontrib>Senapati, K</creatorcontrib><creatorcontrib>Serfass, B</creatorcontrib><creatorcontrib>Speller, D</creatorcontrib><creatorcontrib>Stein, M</creatorcontrib><creatorcontrib>Street, J</creatorcontrib><creatorcontrib>Tanaka, H A</creatorcontrib><creatorcontrib>Toback, D</creatorcontrib><creatorcontrib>Underwood, R</creatorcontrib><creatorcontrib>Villano, A N</creatorcontrib><creatorcontrib>von Krosigk, B</creatorcontrib><creatorcontrib>Welliver, B</creatorcontrib><creatorcontrib>Wilson, J S</creatorcontrib><creatorcontrib>Wilson, M J</creatorcontrib><creatorcontrib>Wright, D H</creatorcontrib><creatorcontrib>Yellin, S</creatorcontrib><creatorcontrib>Yen, J J</creatorcontrib><creatorcontrib>SuperCDMS Collaboration</creatorcontrib><creatorcontrib>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</creatorcontrib><creatorcontrib>Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)</creatorcontrib><creatorcontrib>Univ. of South Dakota, Vermillion, SD (United States)</creatorcontrib><creatorcontrib>Pacific Northwest National Laboratory (PNNL), Richland, WA (United States)</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</creatorcontrib><title>Results from the Super Cryogenic Dark Matter Search Experiment at Soudan</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>We report the result of a blinded search for weakly interacting massive particles (WIMPs) using the majority of the SuperCDMS Soudan data set. With an exposure of 1690 kg d, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP-nucleon cross section of 1.4×10^{-44} (1.0×10^{-44}) cm^{2} at 46 GeV/c^{2}. These results set the strongest limits for WIMP-germanium-nucleus interactions for masses >12 GeV/c^{2}.</description><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNpNkN9P2zAQgC20CQrjX0AWT3tJd04cx35EXVmROjHR7dlyLpc10CbFdtD638-sZeLppLvvfn2MXQmYCgHFlx_rfXiglyXFOBU5TEEJDfkJmwioTFYJIT-wCUAhMgNQnbHzEB4BQORKn7Kz3Egt8qKasMUDhXETA2_9sOVxTXw17sjzmd8Pv6nvkH91_ol_dzGm7IqcxzWf_0lIt6U-chf5ahgb139iH1u3CXR5jBfs1-3852yRLe-_3c1ulhnKMo-ZQmOcUkKqFgw63UJJAhokUrqsdY6aoMQSa2NSDWSDpm1kmw6vK6nRFRfs-jB3CLGzAbtIuMah7wmjFTJPP8oEfT5AOz88jxSi3XYBabNxPQ1jsInSWivxD1UHFP0QgqfW7tJrzu-tAPuq2r5TbZNqe1CdGq-OO8Z6S83_tje3xV_Du3xj</recordid><startdate>20180209</startdate><enddate>20180209</enddate><creator>Agnese, R</creator><creator>Aramaki, T</creator><creator>Arnquist, I J</creator><creator>Baker, W</creator><creator>Balakishiyeva, 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C</creatorcontrib><creatorcontrib>Kelsey, M H</creatorcontrib><creatorcontrib>Kennedy, A</creatorcontrib><creatorcontrib>Kubik, A</creatorcontrib><creatorcontrib>Kurinsky, N A</creatorcontrib><creatorcontrib>Loer, B</creatorcontrib><creatorcontrib>Lopez Asamar, E</creatorcontrib><creatorcontrib>Lukens, P</creatorcontrib><creatorcontrib>MacDonell, D</creatorcontrib><creatorcontrib>Mahapatra, R</creatorcontrib><creatorcontrib>Mandic, V</creatorcontrib><creatorcontrib>Mast, N</creatorcontrib><creatorcontrib>Miller, E H</creatorcontrib><creatorcontrib>Mirabolfathi, N</creatorcontrib><creatorcontrib>Mohanty, B</creatorcontrib><creatorcontrib>Morales Mendoza, J D</creatorcontrib><creatorcontrib>Nelson, J</creatorcontrib><creatorcontrib>Orrell, J L</creatorcontrib><creatorcontrib>Oser, S M</creatorcontrib><creatorcontrib>Page, K</creatorcontrib><creatorcontrib>Page, W A</creatorcontrib><creatorcontrib>Partridge, R</creatorcontrib><creatorcontrib>Penalver Martinez, M</creatorcontrib><creatorcontrib>Pepin, M</creatorcontrib><creatorcontrib>Phipps, A</creatorcontrib><creatorcontrib>Poudel, S</creatorcontrib><creatorcontrib>Pyle, M</creatorcontrib><creatorcontrib>Qiu, H</creatorcontrib><creatorcontrib>Rau, W</creatorcontrib><creatorcontrib>Redl, P</creatorcontrib><creatorcontrib>Reisetter, A</creatorcontrib><creatorcontrib>Reynolds, T</creatorcontrib><creatorcontrib>Roberts, A</creatorcontrib><creatorcontrib>Robinson, A E</creatorcontrib><creatorcontrib>Rogers, H E</creatorcontrib><creatorcontrib>Saab, T</creatorcontrib><creatorcontrib>Sadoulet, B</creatorcontrib><creatorcontrib>Sander, J</creatorcontrib><creatorcontrib>Schneck, K</creatorcontrib><creatorcontrib>Schnee, R W</creatorcontrib><creatorcontrib>Scorza, S</creatorcontrib><creatorcontrib>Senapati, K</creatorcontrib><creatorcontrib>Serfass, B</creatorcontrib><creatorcontrib>Speller, D</creatorcontrib><creatorcontrib>Stein, M</creatorcontrib><creatorcontrib>Street, J</creatorcontrib><creatorcontrib>Tanaka, H A</creatorcontrib><creatorcontrib>Toback, D</creatorcontrib><creatorcontrib>Underwood, R</creatorcontrib><creatorcontrib>Villano, A N</creatorcontrib><creatorcontrib>von Krosigk, B</creatorcontrib><creatorcontrib>Welliver, B</creatorcontrib><creatorcontrib>Wilson, J S</creatorcontrib><creatorcontrib>Wilson, M J</creatorcontrib><creatorcontrib>Wright, D H</creatorcontrib><creatorcontrib>Yellin, S</creatorcontrib><creatorcontrib>Yen, J J</creatorcontrib><creatorcontrib>SuperCDMS Collaboration</creatorcontrib><creatorcontrib>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</creatorcontrib><creatorcontrib>Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)</creatorcontrib><creatorcontrib>Univ. of South Dakota, Vermillion, SD (United States)</creatorcontrib><creatorcontrib>Pacific Northwest National Laboratory (PNNL), Richland, WA (United States)</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Agnese, R</au><au>Aramaki, T</au><au>Arnquist, I J</au><au>Baker, W</au><au>Balakishiyeva, D</au><au>Banik, S</au><au>Barker, D</au><au>Basu Thakur, R</au><au>Bauer, D A</au><au>Binder, T</au><au>Bowles, M A</au><au>Brink, P L</au><au>Bunker, R</au><au>Cabrera, B</au><au>Caldwell, D O</au><au>Calkins, R</au><au>Cartaro, C</au><au>Cerdeño, D G</au><au>Chang, Y</au><au>Chen, Y</au><au>Cooley, J</au><au>Cornell, B</au><au>Cushman, P</au><au>Daal, M</au><au>Di Stefano, P C F</au><au>Doughty, T</au><au>Fascione, E</au><au>Figueroa-Feliciano, E</au><au>Fritts, M</au><au>Gerbier, G</au><au>Germond, R</au><au>Ghaith, M</au><au>Godfrey, G L</au><au>Golwala, S R</au><au>Hall, J</au><au>Harris, H R</au><au>Hong, Z</au><au>Hoppe, E W</au><au>Hsu, L</au><au>Huber, M E</au><au>Iyer, V</au><au>Jardin, D</au><au>Jastram, A</au><au>Jena, C</au><au>Kelsey, M H</au><au>Kennedy, A</au><au>Kubik, A</au><au>Kurinsky, N A</au><au>Loer, B</au><au>Lopez Asamar, E</au><au>Lukens, P</au><au>MacDonell, D</au><au>Mahapatra, R</au><au>Mandic, V</au><au>Mast, N</au><au>Miller, E H</au><au>Mirabolfathi, N</au><au>Mohanty, B</au><au>Morales Mendoza, J D</au><au>Nelson, J</au><au>Orrell, J L</au><au>Oser, S M</au><au>Page, K</au><au>Page, W A</au><au>Partridge, R</au><au>Penalver Martinez, M</au><au>Pepin, M</au><au>Phipps, A</au><au>Poudel, S</au><au>Pyle, M</au><au>Qiu, H</au><au>Rau, W</au><au>Redl, P</au><au>Reisetter, A</au><au>Reynolds, T</au><au>Roberts, A</au><au>Robinson, A E</au><au>Rogers, H E</au><au>Saab, T</au><au>Sadoulet, B</au><au>Sander, J</au><au>Schneck, K</au><au>Schnee, R W</au><au>Scorza, S</au><au>Senapati, K</au><au>Serfass, B</au><au>Speller, D</au><au>Stein, M</au><au>Street, J</au><au>Tanaka, H A</au><au>Toback, D</au><au>Underwood, R</au><au>Villano, A N</au><au>von Krosigk, B</au><au>Welliver, B</au><au>Wilson, J S</au><au>Wilson, M J</au><au>Wright, D H</au><au>Yellin, S</au><au>Yen, J J</au><aucorp>SuperCDMS Collaboration</aucorp><aucorp>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</aucorp><aucorp>Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)</aucorp><aucorp>Univ. of South Dakota, Vermillion, SD (United States)</aucorp><aucorp>Pacific Northwest National Laboratory (PNNL), Richland, WA (United States)</aucorp><aucorp>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Results from the Super Cryogenic Dark Matter Search Experiment at Soudan</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2018-02-09</date><risdate>2018</risdate><volume>120</volume><issue>6</issue><spage>061802</spage><epage>061802</epage><pages>061802-061802</pages><artnum>061802</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>We report the result of a blinded search for weakly interacting massive particles (WIMPs) using the majority of the SuperCDMS Soudan data set. With an exposure of 1690 kg d, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP-nucleon cross section of 1.4×10^{-44} (1.0×10^{-44}) cm^{2} at 46 GeV/c^{2}. These results set the strongest limits for WIMP-germanium-nucleus interactions for masses >12 GeV/c^{2}.</abstract><cop>United States</cop><pub>American Physical Society (APS)</pub><pmid>29481237</pmid><doi>10.1103/PhysRevLett.120.061802</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2018-02, Vol.120 (6), p.061802-061802, Article 061802 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1420014 |
| source | American Physical Society Journals; EZB-FREE-00999 freely available EZB journals |
| subjects | PHYSICS OF ELEMENTARY PARTICLES AND FIELDS |
| title | Results from the Super Cryogenic Dark Matter Search Experiment at Soudan |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-21T18%3A00%3A39IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Results%20from%20the%20Super%20Cryogenic%20Dark%20Matter%20Search%20Experiment%20at%20Soudan&rft.jtitle=Physical%20review%20letters&rft.au=Agnese,%20R&rft.aucorp=SuperCDMS%20Collaboration&rft.date=2018-02-09&rft.volume=120&rft.issue=6&rft.spage=061802&rft.epage=061802&rft.pages=061802-061802&rft.artnum=061802&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.120.061802&rft_dat=%3Cproquest_osti_%3E2008886114%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2008886114&rft_id=info:pmid/29481237&rfr_iscdi=true |